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PBHBeta, a code to explore the constraints on PBH abundances and power spectrum.

Project description

PBH-{math}\beta, a code to explore the constraints on PBH abundances and power spectrum.

Authors: Tadeo D. Gómez & Luis E. Padilla

Source: Source code at GitHub

Licence: GNU General Public License v2.0. The documentation is licensed under the GFDL.

PyPI version License: GPL v2 Documentation Status arXiv


The PBHBeta library is a computational tool designed to calculate constraints on the abundance of Primordial Black Holes (PBHs) and the power spectrum (PS) in cosmological scenarios featuring a non-standard evolution phase between the end of inflation and Big Bang Nucleosynthesis (BBN).

This project is under development.
This code has been tested exclusively with Python version 3.9, and we strongly recommend using it with versions higher than this (Python 3.x and above).

The GitHub repository and PyPI package for PBHBeta include the essential libraries necessary to run PBHBeta. However, these dependencies must be imported into the notebook or console for the functions to become accesible. Refer to the Requeriments and installation sections.

How to cite us

If you use PBH-{math}\beta, please cite arXiv: 2308.04642v1.

Changelog

Versions:

  • 1.0.1 (14/08/2023) Changes were implemented in the names of modules, functions, and classes.
  • 1.0 (05/08/2023) Initial version.

TO-Do

  • Complete the description into documentation to modules and components.

UNAM{.bg-warning w=100px h=130px} ICF{.bg-warning w=250px h=130px} ICTP{.bg-warning w=130px h=130px} CONAHCYT{.bg-warning w=190px h=130px}

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